On the Milankovitch orbital elements for perturbed Keplerian motion

DOI10.1007/S10569-013-9530-7zbMath1298.70017OpenAlexW2006973005MaRDI QIDQ468553

Aaron J. Rosengren, Daniel J. Scheeres

Publication date: 7 November 2014

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10569-013-9530-7

zbMATH Keywords

Kepler problemaveragingvariation of parameterssolar radiation pressurenonsingular elementsorbit perturbation

Mathematics Subject Classification ID

Celestial mechanics (70F15) Orbital mechanics (70M20) Averaging of perturbations for nonlinear problems in mechanics (70K65)

Related Items (7)

Nonsingular vectorial reformulation of the short-period corrections in Kozai's oblateness solution ⋮ Milankovitch equations with spinors ⋮ Hamiltonian reduction through explicit canonical transformations and resonant canonical variables ⋮ Secular dynamics around small bodies with solar radiation pressure ⋮ Uniform formulation for orbit computation: the intermediate elements ⋮ Lunar close encounters compete with the circumterrestrial Lidov-Kozai effect. The dynamical demise of \textit{Luna 3} ⋮ A vectorial approach to determine frozen orbital conditions

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